2,017 research outputs found
Interpretation of High Energy String Scattering in terms of String Configurations
High energy string scattering at fixed momentum transfer, known to be
dominated by Regge trajectory exchange, is interpreted by identifying families
of string states which induce each type of trajectory exchange. These include
the usual leading trajectory and its daughters as
well as the ``sister'' trajectories and their
daughters. The contribution of the sister to high energy scattering
is dominated by string excitations in the mode. Thus, at large ,
string scattering is dominated by wee partons, consistently with a picture of
string as an infinitely composite system of ``constituents'' which carry zero
energy and momentum.Comment: 14 pages, phyzzx, psfig required, Florida Preprint UFIFT-94-
Minimal Length Uncertainty Relation and the Hydrogen Spectrum
Modifications of Heisenberg's uncertainty relations have been proposed in the
literature which imply a minimum position uncertainty. We study the low energy
effects of the new physics responsible for this by examining the consequent
change in the quantum mechanical commutation relations involving position and
momenta. In particular, the modifications to the spectrum of the hydrogen atom
can be naturally interpreted as a varying (with energy) fine structure
constant. From the data on the energy levels we attempt to constrain the scale
of the new physics and find that it must be close to or larger than the weak
scale. Experiments in the near future are expected to change this bound by at
least an additional order of magnitude.Comment: 8 pages, no figure. Corrected typos, added a reference with comment
Gamma-Ray Bursts and Dark Energy - Dark Matter interaction
In this work Gamma Ray Burst (GRB) data is used to place constraints on a
putative coupling between dark energy and dark matter. Type Ia supernovae (SNe
Ia) constraints from the Sloan Digital Sky Survey II (SDSS-II) first-year
results, the cosmic microwave background radiation (CMBR) shift parameter from
WMAP seven year results and the baryon acoustic oscillation (BAO) peak from the
Sloan Digital Sky Survey (SDSS) are also discussed. The prospects for the field
are assessed, as more GRB events become available.Comment: 7 pages, 3 figures. Version to match the one published in Mon. Not.
R. Ast. So
Classicalization of Gravitons and Goldstones
We establish a close parallel between classicalization of gravitons and
derivatively-coupled Nambu-Goldstone-type scalars. We show, that black hole
formation in high energy scattering process represents classicalization with
the classicalization radius given by Schwarzschild radius of center of mass
energy, and with the precursor of black hole entropy being given by number of
soft quanta composing this classical configuration. Such an entropy-equivalent
is defined for scalar classicalons also and is responsible for exponential
suppression of their decay into small number of final particles. This parallel
works in both ways. For optimists that are willing to hypothesize that gravity
may indeed self-unitarize at high energies via black hole formation, it
illustrates that the Goldstones may not be much different in this respect, and
they classicalize essentially by similar dynamics as gravitons. In the other
direction, it may serve as an useful de-mystifier of
via-black-hole-unitarization process and of the role of entropy in it, as it
illustrates, that much more prosaic scalar theories essentially do the same.
Finally, it illustrates that in both cases classicalization is the defining
property for unitarization, and that it sets-in before one can talk about
accompanying properties, such as entropy and thermality of static classicalons
(black holes). These properties are by-products of classicalization, and their
equivalents can be defined for non-gravitational cases of classicalization.Comment: 23 page
On the Zero-Slope Limit of the Compactified Closed Bosonic String
In the framework of the compactified closed bosonic string theory with the
extra spatial coordinates being circular with radius , we perform both the
zero-slope limit and the limit of the tree scattering
amplitude of four massless scalar particles. We explicitly show that this
double limit leads to amplitudes involving scalars which interact through the
exchange of a scalar, spin 1 and spin 2 particle. In particular, this latter
case reproduces the same result obtained in linearized quantum gravity.Comment: 10 pages, LaTex file, DSF-T-43/9
Supersymmetry, the Cosmological Constant and a Theory of Quantum Gravity in Our Universe
There are many theories of quantum gravity, depending on asymptotic boundary
conditions, and the amount of supersymmetry. The cosmological constant is one
of the fundamental parameters that characterize different theories. If it is
positive, supersymmetry must be broken. A heuristic calculation shows that a
cosmological constant of the observed size predicts superpartners in the TeV
range. This mechanism for SUSY breaking also puts important constraints on low
energy particle physics models. This essay was submitted to the Gravity
Research Foundation Competition and is based on a longer article, which will be
submitted in the near future
Teaching a New Dog Old Tricks: Resurrecting Multilingual Retrieval Using Zero-shot Learning
While billions of non-English speaking users rely on search engines every
day, the problem of ad-hoc information retrieval is rarely studied for
non-English languages. This is primarily due to a lack of data set that are
suitable to train ranking algorithms. In this paper, we tackle the lack of data
by leveraging pre-trained multilingual language models to transfer a retrieval
system trained on English collections to non-English queries and documents. Our
model is evaluated in a zero-shot setting, meaning that we use them to predict
relevance scores for query-document pairs in languages never seen during
training. Our results show that the proposed approach can significantly
outperform unsupervised retrieval techniques for Arabic, Chinese Mandarin, and
Spanish. We also show that augmenting the English training collection with some
examples from the target language can sometimes improve performance.Comment: ECIR 2020 (short
Hamiltonian BRST Quantization of the Conformal String
We present a new formulation of the tensionless string () where the
space-time conformal symmetry is manifest. Using a Hamiltonian BRST scheme we
quantize this {\em Conformal String} and find that it has critical dimension
. This is in keeping with our classical result that the model describes
massless particles in this dimension. It is also consistent with our previous
results which indicate that quantized conformally symmetric tensionless strings
describe a topological phase away {}from . We reach our result by
demanding nilpotency of the BRST charge and consistency with the Jacobi
identities. The derivation is presented in two different ways: in operator
language and using mode expansions. Careful attention is payed to
regularization, a crucial ingredient in our calculations.Comment: 33pp (LaTeX), USITP-94-0
Prospects for multi-messenger extended emission from core-collapse supernovae in the Local Universe
Multi-messenger emissions from SN1987A and GW170817/GRB170817A suggest a
Universe rife with multi-messenger transients associated with black holes and
neutron stars. For LIGO-Virgo, soon to be joined by KAGRA, these observations
promise unprecedented opportunities to probe the central engines of
core-collapse supernovae (CC-SNe) and gamma-ray bursts. Compared to neutron
stars, central engines powered by black hole-disk or torus systems may be of
particular interest to multi-messenger observations by the relatively large
energy reservoir of angular momentum, up to 29\% of total mass in the
Kerr metric. These central engines are expected from relatively massive stellar
progenitors and compact binary coalescence involving a neutron star. We review
prospects of multi-messenger emission by catalytic conversion of by a
non-axisymmetric disk or torus. Observational support for this radiation
process is found in a recent identification of in Extended Emission to GW170817 at a significance of
4.2\, concurrent with GRB170817A. A prospect on similar emissions from
nearby CC-SNe justifies the need for all-sky blind searches of long duration
bursts by heterogeneous computing.Comment: 96 pages, 20 figure
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